Astrophysics > Earth and Planetary Astrophysics

Title:A Super-Earth Orbiting the Nearby Sun-like Star HD 1461

Abstract: We present precision radial velocity data that reveal a Super-Earth mass
planet and two probable additional planets orbiting the bright nearby G0V star
HD 1461. Our 12.8 years of Keck HIRES precision radial velocities indicate the
presence of a 7.4M_Earth planet on a 5.77-day orbit. The data also suggest, but
cannot yet confirm, the presence of outer planets on low-eccentricity orbits
with periods of 446.1 and 5017 days, and projected masses (M sin i) of 27.9 and
87.1M_Earth, respectively. Test integrations of systems consistent with the
radial velocity data suggest that the configuration is dynamically stable. We
present a 12.2-year time series of photometric observations of HD 1461, which
comprise 799 individual measurements, and indicate that it has excellent
long-term photometric stability. However, there are small amplitude variations
with periods comparable to those of the suspected 2nd and 3rd signals in the
radial velocities near 5000 and 446 days, thus casting some suspicion on those
periodicities as Keplerian signals. If the 5.77-day companion has a
Neptune-like composition, then its expected transit depth is of order ~0.5
millimags. The geometric a priori probability of transits is ~8%. Phase-folding
of the ground-based photometry shows no indication that transits of the
5.77-day companion are occurring, but high-precision follow-up of HD 1461
during upcoming transit phase windows will be required to definitively rule out
or confirm transits. This new system joins a growing list of solar-type stars
in the immediate galactic neighborhood that are accompanied by at least one
Neptune- (or lower) mass planets having orbital periods of 50 days or less.